Superconducting Chevrel phase PbMo$_{6}$S$_{8}$ from first principles

TL;DR

This paper uses first-principles calculations to analyze the superconducting properties of PbMo$_{6}$S$_{8}$, revealing strong electron-phonon coupling, the influence of phase instability, and pressure effects on critical temperature.

Contribution

It provides a comprehensive ab initio study of PbMo$_{6}$S$_{8}$, confirming phonon-driven superconductivity and elucidating the role of Coulomb repulsion and pressure dependence.

Findings

Strong electron-phonon coupling near a structural phase transition

Accurate reproduction of critical temperature and gap via SCDFT

Pressure influences on superconducting critical temperature

Abstract

Chevrel ternary superconductors show an intriguing coexistence of molecular aspects, large electron-phonon and electron-electron correlations, which to some extent still impedes their quantitative understanding. We present a first principles study on the prototypical Chevrel compound PbMo$_{6}$S$_{8}$, including electronic, structural and vibrational properties at zero and high pressure. We confirm the presence of an extremely strong electron-phonon coupling, linked to the proximity to a R$\overline{3}$-P$\overline{1}$ structural phase transition, which weakens as the system, upon applied pressures, is driven away from the phase boundary. A detailed description of the superconducting state is obtained by means of fully \textit{ab initio} superconducting density functional theory (SCDFT). SCDFT accounts for the role of phase instability, electron-phonon coupling with different intra- and inter-molecular phonon modes, and without any empirical parameter, and accurately reproduces the experimental critical temperature and gap. This study provides the conclusive confirmation that Chevrel phases are phonon driven superconductors mitigated, however, by an uncommonly strong Coulomb repulsion. The latter is generated by the combined effect of repulsive Mo states at the Fermi energy and a band gap in close proximity to the Fermi level. This is crucial to rationalize why Chevrel phases, in spite of their extreme electron-phonon coupling, have critical temperatures below 15~K. In addition, we predict the evolution of the superconducting critical temperature as a function of the external pressure, showing an excellent agreement with available experimental data.